NASA NTRS · 19950036819
Detection os X-rays from SN 1993J with ASCA
Abstract
ASCA observed SN 1993J seven times between April 5 and October 24 in 1993. The 1-10 keV luminosity 10d after the explosion was (15 +/- 4) x 10(exp 39) erg/s and decreased monotonicly to (1.3 +/- 0.4) x 10(exp 39) erg/s 210 d after the explosion, when a distance of 3.6 Mpc was assumed. The hardness ratio (2-10 keV/0.5-2 keV) significantly decreased during the course of the observations. The spectrum obtained from a sky region including not only SN 1993J but also the nearby X-ray source clearly shows an iron emission line. The correlation between the iron line flux with the SN 1993J flux suggests that the iron line emission originated in SN 1993J. These observational results are discussed in the context of thermal X-ray emission from a hot region behind the shock due to the collision of the supernova ejecta with the pre-supernova stellar wind.
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Kohmura, Yoshiki, Inoue, Hajime, Aoki, Takashi, Ishida, Manabu, Itoh, Masayuki, Kotani, Taro, Tanaka, Yasuo, Ishisaki, Yoshitaka, Makishima, Kazuo, Matsushita, Kyoko. 1994-01-01. Detection os X-rays from SN 1993J with ASCA. https://ntrs.nasa.gov/citations/19950036819
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